Star Cluster Luminosity Function is a statistical construct in astrophysics that describes the number distribution of star clusters per unit luminosity interval, distinguishing it from related photometric measures by specifically quantifying the abundance of clusters as a function of their intrinsic brightness within a given stellar population.
755
Publications
44.6K
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1.8K
Authors
542
Institutions
Publications per year
2017–2026
68
Variants
Sclf
Parents
Publications
755
1–5 of 755
Authors
1.8K
- WE
21
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- AB
20
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- LF
19
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- JCJean‐Charles Cuillandre
Centre National de la Recherche Scientifique, France
23 publications · 822 citations
18
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- SB
18
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Institutions
542
Space Telescope Science Institute
Baltimore, United States
42 h-index
159 publications
15.3K citations
European Southern Observatory
Garching bei München, Germany
33 h-index
75 publications
4.6K citations
Center for Astrophysics Harvard & Smithsonian
Cambridge, United States
31 h-index
56 publications
4.6K citations
Herzberg Institute of Astrophysics
Victoria, Canada
27 h-index
104 publications
5.2K citations
California Institute of Technology
Pasadena, United States
27 h-index
70 publications
5.3K citations
Johns Hopkins University
Baltimore, United States
27 h-index
61 publications
3.9K citations
Durham University
Durham, United Kingdom
26 h-index
39 publications
3K citations
University of California, Santa Cruz
Santa Cruz, United States
26 h-index
49 publications
3K citations
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- The Astrophysical Journal
ApJ · 221 publications · 15K citations
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- The Astronomical Journal
AJ · 132 publications · 7.7K citations
50
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- Monthly Notices of the Royal Astronomical Society
129 publications · 6.3K citations
48
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- Astronomy and Astrophysics
107 publications · 6.1K citations
42
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- CERN Document Server (European Organization for Nuclear Research)
Repository · 21 publications · 2.2K citations
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